2024RAA....24g5011Z


Query : 2024RAA....24g5011Z

2024RAA....24g5011Z - Research in Astron. and astroph., 24, part no 7, 5011 (2024/July-0)

UWLPIPE: Ultra-wide Bandwidth Low-frequency Pulsar Data Processing Pipeline.

ZHANG Y.-Z., ZHANG H.-L., WANG J., LI J., YE X.-C., WANG S.-Q., DU X., WU H., ZHANG T. and GUO S.-C.

Abstract (from CDS):

For real-time processing of ultra-wide bandwidth low-frequency pulsar baseband data, we designed and implemented an ultra-wide bandwidth low-frequency pulsar data processing pipeline (UWLPIPE) based on the shared ringbuffer and GPU parallel technology. UWLPIPE runs on the GPU cluster and can simultaneously receive multiple 128 MHz dual-polarization VDIF data packets preprocessed by the front-end FPGA. After aligning the dual-polarization data, multiple 128M subband data are packaged into PSRDADA baseband data or multi-channel coherent dispersion filterbank data, and multiple subband filterbank data can be spliced into wideband data after time alignment. We used the Nanshan 26 m radio telescope with the L-band receiver at 964 ∼ 1732 MHz to observe multiple pulsars. Finally, we processed the data using DSPSR software, and the results showed that each subband could correctly fold out the pulse profile, and the wideband pulse profile accumulated by multiple subbands could be correctly aligned.

Abstract Copyright: © 2024. National Astronomical Observatories

Journal keyword(s): (stars:) pulsars: general - methods: data analysis - techniques: miscellaneous

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 PSR B0329+54 Psr 03 32 59.3370698592 +54 34 45.028206408           ~ 690 1
2 PSR B1933+16 Psr 19 35 47.7011639352 +16 16 40.034899524           ~ 328 1
3 PSR B2021+51 Psr 20 22 49.8730 +51 54 50.233           ~ 288 1

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